Constancy of period in TX Ceti

dc.contributor.author	Srivastava, R. K.
dc.date.accessioned	2010-02-02T06:51:24Z
dc.date.available	2010-02-02T06:51:24Z
dc.date.issued	1990
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/483
dc.description.abstract	A slightly improved period (P = 0.ᵈ7408401) of the eclipsing binary system TX Ceti has been given, which is based on all available times of minima. The O-C diagrams based on the period given in PPEN (1980) and based on the new period, have been given. The period of TX Ceti shows fair constancy between the time interval 1928 to 1988. The present O-C diagrams do not confirm, either the presence of a third body or the presence of mass transfer as suggested earlier.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass166-205
dc.subject	TX Ceti	en_US
dc.title	Constancy of period in TX Ceti	en_US
dc.type	Article	en_US